Nonbaryonic' dark matter as baryonic colour superconductor

被引:0
作者
Zhitnitsky, AR [1 ]
机构
[1] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2003年 / 10期
关键词
dark matter; axions;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss a novel cold dark matter candidate which is formed from the ordinary quarks during the QCD phase transition when the axion domain wall undergoes an unchecked collapse due to the tension in the wall. If a large number of quarks is trapped inside the bulk of a closed axion domain wall, the collapse stops due to the internal Fermi pressure. In this case, the system in the bulk may reach the critical density when it undergoes a phase transition to a colour superconducting phase with the ground state being the quark condensate, similar to the Cooper pairs in BCS theory. If this happens, the new state of matter representing the diquark condensate with a large baryon number Bsimilar to10(32) becomes a stable soliton-like configuration. Consequently, it may serve as a novel cold dark matter candidate.
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页数:23
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